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New Estimates of the Solar-Neighborhood Massive Star Birthrate and the Galactic Supernova Rate The birthrate of stars of masses >=10 Msolar is estimatedfrom a sample of just over 400 O3-B2 dwarfs within 1.5 kpc of the Sunand the result extrapolated to estimate the Galactic supernova ratecontributed by such stars. The solar-neighborhood Galactic-plane massivestar birthrate is estimated at ~176 stars kpc-3Myr-1. On the basis of a model in which the Galactic stellardensity distribution comprises a ``disk+central hole'' like that of thedust infrared emission (as proposed by Drimmel and Spergel), theGalactic supernova rate is estimated at probably not less than ~1 normore than ~2 per century and the number of O3-B2 dwarfs within the solarcircle at ~200,000.
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Osservazione e dati astrometrici
Costellazione: | Cane Maggiore |
Ascensione retta: | 06h41m27.48s |
Declinazione: | -24°22'59.0" |
Magnitudine apparente: | 8.259 |
Distanza: | 324.675 parsec |
Moto proprio RA: | -6.8 |
Moto proprio Dec: | 5.5 |
B-T magnitude: | 8.147 |
V-T magnitude: | 8.25 |
Cataloghi e designazioni:
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